The three dimensional theory of gravitation based on a temporal scalar field in Riemanian geometry
S. Kozyrev
Abstract
A new approach to the model of the universe based on work by Rippl, Romero, Tavakol is presented. We have used the scheme for relating the vacuum (D + 1) dimensional theories to D dimensional theories for setting up a correspondence between vacuum 4-dimensional Einstein theory with 3-dimensional gravity theory with temporal scalar field. These ideas we continued by using the 3-dimensional analog of Jordan, Brans-Dicke theory with temporal scalar field. As the result space and time are treated in completely different ways. For the case of a static spherically symmetric field new vacuum static solutions are found.
Create a lesson
Related papers
Testing compact binary nature in eccentric orbits with third-generation detectors
Syed U. Naqvi, Kaushik Paul, Chandra Kant Mishra
Turning Selection Bias into a New Statistic: Asymmetry and Fringes of Lensed Gravitational Waves
Juno C. L. Chan, Elwin K. Y. Li
Exact two-loop gravitational tail integrals and their ultraviolet-infrared structure
Gabriel Luz Almeida
Noncommutative BTZ Gravastar in Gauss-Bonnet Gravity
M. A. Anacleto, A. T. N. Silva, L. Casarini et al.
Mini-Superspace Hamiltonian Dynamics and Canonical Quantization of Bumblebee Cosmology
Pranjal Sarmah
Dynamical stability and observational constraints on a late-time dark-matter particle-creation model
Anirban Chatterjee